- Abstract:
-
Boxy and peanut-shaped bulges are seen in about half of edge-on disc galaxies. Comparisons of the photometry and major-axis gas and stellar kinematics of these bulges to simulations of bar formation and evolution indicate that they are bars viewed in projection. If the properties of boxy bulges can be entirely explained by assuming that they are bars, then this may imply that their hosts are pure disc galaxies with no classical bulge. A handful of these bulges, including that of the Milky Way...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2011.18535.x
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 414
- Issue:
- 3
- Pages:
- 2163-2172
- Publication date:
- 2011-07-05
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:6134eb61-e313-43a9-bcaf-e6964b1ab086
- Source identifiers:
-
170223
- Local pid:
- pubs:170223
- Language:
- English
- Keywords:
- Copyright date:
- 2011
Journal article
The stellar kinematics and populations of boxy bulges: cylindrical rotation and vertical gradients
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